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29
A Discussion of Plausible Solar Irradiance Variations
- Journal of Geophysical Research
, 1993
"... From satellite observations the solar total irradiance is known to vary. Sunspot blocking, facular emission, and network emission are three identified causes for the variations. In this paper we examine several different solar indices measured over the past century that are potential proxy measures ..."
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Cited by 95 (0 self)
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From satellite observations the solar total irradiance is known to vary. Sunspot blocking, facular emission, and network emission are three identified causes for the variations. In this paper we examine several different solar indices measured over the past century that are potential proxy measures for the Sun's irradiance. These indices are (1) the equatorial solar rotation rate, (2) the sunspot structure, the decay rate of individual sunspots, and the number of sunspots without umbrae, and (3) the length and decay rate of the sunspot cycle. Each index can be used to develop a model for the Sun's total irradiance as seen at the Earth. Three solar indices allow the irradiance to be modeled back to the mid-1700s. The indices are (1) the length of the solar cycle, (2) the normalized decay rate of the solar cycle, and (3) the mean level of solar activity. All the indices are well correlated, and one possible explanation for their nearly simultaneous variations is changes in the Sun's convective energy transport. Although changes in the Sun's convective energy transport are outside the realm of normal stellar structure theory (e.g., mixing length theory), one can imagine variations arising from even the simplest view of sunspots as vertical tubes of magnetic flux, which would serve as rigid pillars affecting the energy flow patterns by ensuring larger-scale eddies. A composite solar irradiance model, based upon these proxies, is compared to the northern hemisphere temperature departures for 1700-1992.
Response of global upper ocean temperature to changing solar irradiance
- Journal of Geophysical Research
, 1997
"... Abstract. By focusing on time sequences of basin-average and global-average upper ocean temperature (i.e., from 40øS to 60øN) we find temperatures responding to changing solar irradiance in three separate frequency bands with periods of>100 years, 18-25 years, and 9-13 years. Moreover, we find th ..."
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Cited by 73 (2 self)
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Abstract. By focusing on time sequences of basin-average and global-average upper ocean temperature (i.e., from 40øS to 60øN) we find temperatures responding to changing solar irradiance in three separate frequency bands with periods of>100 years, 18-25 years, and 9-13 years. Moreover, we find them in two different data sets, that is, surface marine weather observations from 1990 to 1991 and bathythermograph (BT) upper ocean temperature profiles from 1955 to 1994. Band-passing basin-average temperature records find each frequency component in phase across the Indian, Pacific, and Atlantic Oceans, yielding global-average records with maximum amplitudes of 0.04 ø _+ 0.01øK and 0.07 ø _+ 0.01øK on decadal and interdecadal scales, respectively. These achieve maximum correlation with solar irradiance records (i.e., with maximum amplitude 0.5 W m-2 at the top of the atmosphere) at phase lags ranging from 30 ø to 50 ø. From the BT data set, solar signals in global-average temperature penetrate to 80-160 m, confined to the upper layer above the main pycnocline. Operating a global-average heat budget for the upper ocean yields sea surface temperature responses of 0.01ø-0.03øK and 0.02ø-0.05øK on decadal and interdecadal scales, respectively, from the 0.1 W m-2 penetration of solar irradiance to the sea surface. Since this is of the same order as that observed (i.e., 0.04ø-0.07øK), we can infer that anomalous heat from changing solar irradiance is stored in the upper layer of the ocean. 1.
Sardine and anchovy regime fluctuations of abundance in four regions of the world oceans: a workshop report
, 1992
"... Regimes of high abundance of sardine (Sardinops sagax and sardina pikhardw) have alternated with regimes of high abundance of anchovy (Engradis spp.) in each of the five regions of the world where these taxa co-occur and have been extensively fished. When one taxon has been plentiful, the other has ..."
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Cited by 24 (0 self)
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Regimes of high abundance of sardine (Sardinops sagax and sardina pikhardw) have alternated with regimes of high abundance of anchovy (Engradis spp.) in each of the five regions of the world where these taxa co-occur and have been extensively fished. When one taxon has been plentiful, the other has usually been at a reduced level of abundance, and vice versa. Changes in the four heavily fished regions that support S. sagax-the Japanese, Californian, Humboldt, and Benguela sys-tems-from a regime dominated by one taxon to a high level of abundance of the other have occurred more or less simultaneously. In the Pacific Ocean, sardines have tended to increase during periods of increasing global air and sea temperatures and anchovies to de-
Holocene environmental and climatic change in the Northern Great Plains as recorded in the geochemistry of sediments
- in Pickerel Lake, South Dakota. Quaternary International
"... Holocene environmental and climatic change in the Northern Great Plains as recorded in the geochemistry of sediments in Pickerel Lake, ..."
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Cited by 12 (2 self)
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Holocene environmental and climatic change in the Northern Great Plains as recorded in the geochemistry of sediments in Pickerel Lake,
2005: Externally forced and internal variability in ensemble climate simulations of the Maunder Minimum
- J. Clim
"... The response of the climate system to natural, external forcing during the Maunder Minimum (ca. A.D. 1645–1715) is investigated using a comprehensive climate model. An ensemble of six transient simulations is produced in order to examine the relative importance of externally forced and internally ge ..."
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Cited by 8 (1 self)
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The response of the climate system to natural, external forcing during the Maunder Minimum (ca. A.D. 1645–1715) is investigated using a comprehensive climate model. An ensemble of six transient simulations is produced in order to examine the relative importance of externally forced and internally generated variability. The simulated annual Northern Hemisphere and zonal-mean near-surface air temperature agree well with proxy-based reconstructions on decadal time scales. A mean cooling signal during the Maunder Minimum is masked by the internal unforced variability in some regions such as Alaska, Greenland, and northern Europe. In general, temperature exhibits a better signal-to-noise ratio than precipitation. Mean salinity changes are found in basin averages. The model also shows clear response patterns to volcanic eruptions. In particular, volcanic forcing is projected onto the winter North Atlantic Oscillation index following the eruptions. It is demonstrated that the significant spread of ensemble members is possible even on multidecadal time scales, which has an important implication in coordinating comparisons between
Persistence of the Gleissberg 88-year solar cycle over the last ˜12,000years: Evidence from cosmogenic isotopes
- J. Geoph. Res
"... [1] Among other longer-than-22-year periods in Fourier spectra of various solar– terrestrial records, the 88-year cycle is unique, because it can be directly linked to the cyclic activity of sunspot formation. Variations of amplitude as well as of period of the Schwabe 11-year cycle of sunspot activ ..."
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Cited by 6 (0 self)
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[1] Among other longer-than-22-year periods in Fourier spectra of various solar– terrestrial records, the 88-year cycle is unique, because it can be directly linked to the cyclic activity of sunspot formation. Variations of amplitude as well as of period of the Schwabe 11-year cycle of sunspot activity have actually been known for a long time and a ca. 80-year cycle was detected in those variations. Manifestations of such secular periodic processes were reported in a broad variety of solar, solar–terrestrial, and terrestrial climatic phenomena. Confirmation of the existence of the Gleissberg cycle in long solar– terrestrial records as well as the question of its stability is of great significance for solar dynamo theories. For that perspective, we examined the longest detailed cosmogenic isotope record—INTCAL98 calibration record of atmospheric 14C abundance. The most detailed precisely dated part of the record extends back to 11,854 years B.P. During this whole period, the Gleissberg cycle in 14C concentration has a period of 87.8 years and an average amplitude of 1 % (in 14C units). Spectral analysis indicates in frequency domain by sidebands of the combination tones at periods of 91.5 ± 0.1 and 84.6 ± 0.1 years that the amplitude of the Gleissberg cycle appears to be modulated by other long-
2001: Solar variability and climate
- J. Geophys. Res
"... Abstract. Recent precise observations of solar global parameters are used to calibrate an upgraded solar model which takes into account magnetic fields in the solar interior. Historical data about sunspot numbers (from 1500 to the present) and solar radius changes (between 1715 and 1979) are used to ..."
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Abstract. Recent precise observations of solar global parameters are used to calibrate an upgraded solar model which takes into account magnetic fields in the solar interior. Historical data about sunspot numbers (from 1500 to the present) and solar radius changes (between 1715 and 1979) are used to compute solar variability on years to centuries timescales. The results show that although the 11 year variability of the total irradiance is of the order of 0.1%, additional, longer lived changes of the order of 0.1 % may have occurred in the past centuries. These could, for example, account for the occurrence of climate excursions such as little ice ages.
unknown title
, 2005
"... Climate variability in Scandinavia for the past millennium simulated by an atmosphere-ocean general circulation model ..."
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Climate variability in Scandinavia for the past millennium simulated by an atmosphere-ocean general circulation model
3745 Resonant Interactions between Solar Activity and Climate
"... ABSTRACT Solar magnetic activity exhibits chaotically modulated cycles with a mean period of 11 yr, which are responsible for slight variations in solar luminosity and modulation of the solar wind, while the earth's atmosphere and oceans support oscillations with many different frequencies. Al ..."
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ABSTRACT Solar magnetic activity exhibits chaotically modulated cycles with a mean period of 11 yr, which are responsible for slight variations in solar luminosity and modulation of the solar wind, while the earth's atmosphere and oceans support oscillations with many different frequencies. Although there are several mechanisms that might couple solar variability with climate, there is, as yet, no compelling evidence that a direct forcing is sufficiently effective to drive climatic change. In many nonlinear systems resonant coupling allows weak forcing to have a dramatic effect. An idealized model is considered, in which the solar dynamo and the climate are represented by low-order systems, each of which in isolation supports chaotic oscillations. The climate is represented by the Lorenz equations: solutions oscillate about either of two fixed points, representing warm and cold states, flipping sporadically between them. The effect of a weak nonlinear input from the dynamo to the climate that tends to push it toward the warm state is computed. This input has a significant effect when the ''typical frequencies'' of each system are in resonance. The solution is now asymmetric, with the warm state preferred. The degree of asymmetry is less than might be anticipated, because resonant forcing extends the duration of oscillations about either state, and so increases the timescale for flipping. The presence of grand minima in the solar output leads to complicated intermittent behavior in the climate. Consequently, the results of frequency analysis are sensitive to the duration of time series that is used. It is clear that the resonance provides a powerful mechanism for amplifying climate forcing by solar activity.
Identification
, 2002
"... of a change in climate state using regional flood data ..."
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